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White Dwarfs in the HET Dark Energy Experiment Bárbara G. Castanheira The University of Texas at Austin Universität Wien 17 th European White Dwarf Workshop – Tübingen, August 16-20, 2010

White Dwarfs in the HET Dark Energy Experiment

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17 th European White Dwarf Workshop – Tübingen , August 16-20, 2010 . White Dwarfs in the HET Dark Energy Experiment. Bárbara G. Castanheira. The University of Texas at Austin Universität Wien. 17 th European White Dwarf Workshop – Tübingen , August 16-20, 2010 . - PowerPoint PPT Presentation

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Page 1: White Dwarfs in the  HET Dark Energy Experiment

White Dwarfs in the HET Dark Energy Experiment

Bárbara G. Castanheira

The University of Texas at AustinUniversität Wien

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Page 2: White Dwarfs in the  HET Dark Energy Experiment

Hobby-Eberly Telescope

Location: McDonald Observatory (30° 40' N)

Low cost: 15-20% of the cost of a 9 m telescope

Primary mirror: 11.1 x 9.8 m (9.2 m effective aperture)

91 hexagonal mirrors

Fixed elevation angle of 55o (tilted Arecibo design)

Access 81% of the sky

Queue schedule

Instruments: HRS, LRS, MRS

Model for SALT

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Page 3: White Dwarfs in the  HET Dark Energy Experiment

HETDEX: HET Dark Energy Experiment

Goal: probe dark energy

Observations: ~ 1400 hours in 3 years

Technique: expansion of the universe at 0<z<4

Main targets: Lyman-α emitting galaxies

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

(Hill et al. 2008)

Page 4: White Dwarfs in the  HET Dark Energy Experiment

Dark energy:

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Supernovae discovery of accelerated expansion

Within GR: smooth energy with large negative pressure

75% of the universe

Acceleration began at z~0.4 and t~10Gyr

Page 5: White Dwarfs in the  HET Dark Energy Experiment

(Frieman et al. 2008)

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Page 6: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Destiny of the universe depends critically upon the nature of dark energy!

Page 7: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX field:

Page 8: White Dwarfs in the  HET Dark Energy Experiment

VIRUS-P Review: Visual Integral-field Replicable Unit

Spectrograph - Prototype

1.9’x1.9’ FOV at 2.7 m HJST

1/3 fill factor

Largest FOV of any existing IFU

4.2’’ diameter fibers on sky

3500-5800Å wavelength range

R=1000 @ 5000Å

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Page 9: White Dwarfs in the  HET Dark Energy Experiment

Flux calibrating the pilot survey:17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Feige 34

Page 10: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 1:

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17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 2:

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17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 3:

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17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 4:

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17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 5:

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17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Dither 6:

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17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Feige 34:

VIRUS-P

2.7m HJST

6x120s

V=11.2

Page 17: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX details:150 VIRUS3500-5500Å~3400 spectraFOV 22arcminResolution ~5Å~140 nights, 3 years

PARALLEL SURVEY

Page 18: White Dwarfs in the  HET Dark Energy Experiment

(Drory 2010)

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

Page 19: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

White Dwarfs in HETDEX

~20000 White Dwarfs Magnitude limited sample For V=22, S/N=3 Main and Parallel surveys

A powerful survey!

Page 20: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

HETDEX current status:

Schedule: late 2011 VIRUS-P at HET Replication of spectrographs Software (CURE or VACCINE & DIAGNOSE) Additional science

Page 21: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

White dwarf science goals:

WD Luminosity Function New candidates of pulsators (2.1m) New “flavors” of WDs?

Page 22: White Dwarfs in the  HET Dark Energy Experiment

17th European White Dwarf Workshop – Tübingen, August 16-20, 2010

[email protected]

Danke! Obrigada!